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Search for Nonstandard Neutrino Interactions with IceCube DeepCore

As atmospheric neutrinos propagate through the Earth, vacuumlike oscillations are modified by Standard Model neutral- and charged-current interactions with electrons. Theories beyond the Standard Model introduce heavy, TeV-scale bosons that can produce nonstandard neutrino interactions. These additi...

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Main Authors: Ahrens, M., Al Samarai, I., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Axani, S., Bai, X., Barron, J. P., Barwick, S. W., Becker Tjus, J., Binder, G., Bindig, D., Bose, D., Bourbeau, E., Bourbeau, J., Bradascio, F., Brayeur, L., Brenzke, M., Bron, S., Cheung, E., Christov, A., Collin, G. H., Cowen, D. F., Cross, R., De André, J. P. A. M., DeLaunay, J. J., Desiati, P., Ehrhardt, T., Eichmann, B., Eller, P., Fazely, A. R., Friedman, E., Fuchs, T., Giang, W., Goldschmidt, A., Helbing, K., Hickford, S., Hoffmann, R., Huber, M., In, S., Jacobi, E., Japaridze, G. S., Jeong, M., Jones, B. J. P., Karle, A., Katz, U., Kelley, J. L., Kheirandish, A., Kirby, C., Kohnen, G., Kolanoski, H., Köpke, L., Kopper, C., Kroll, M., Krückl, G., Kunwar, Samridha, Meagher, K., Meier, M., Momenté, G., Montaruli, T., Moore, R. W., Nahnhauer, R., Nygren, D. R., O'Murchadha, A., Palczewski, T., Pérez De Los Heros, C., Pieloth, D., Price, P. B., Raab, C., Rawlins, K., Reimann, R., Rongen, M., Sälzer, T., Sandroos, J., Santander, M., Schoenen, S., Soedingrekso, J., Stachurska, J., Stanev, T., Stokstad, R. G., Tenholt, F., Tosi, D., Tselengidou, M., Turcati, A., Van Eijndhoven, N., Vehring, M., Vogel, E., Wallraff, M., Wandler, F. D., Waza, A., Werthebach, J., Westerhoff, S., Wille, L., Wills, L., Yanez, J. P., Yodh, G., Yoshida, S., Yuan, T., Zoll, M.
Format: Report
Language:English
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Summary:As atmospheric neutrinos propagate through the Earth, vacuumlike oscillations are modified by Standard Model neutral- and charged-current interactions with electrons. Theories beyond the Standard Model introduce heavy, TeV-scale bosons that can produce nonstandard neutrino interactions. These additional interactions may modify the Standard Model matter effect producing a measurable deviation from the prediction for atmospheric neutrino oscillations. The result described in this paper constrains nonstandard interaction parameters, building upon a previous analysis of atmospheric muon-neutrino disappearance with three years of IceCube DeepCore data. The best fit for the muon to tau flavor changing term is εμτ=-0.0005, with a 90% C.L. allowed range of -0.0067
ISSN:1550-7998
1538-4500
2470-0029
0556-2821
2470-0010
1089-4918
1550-2368
DOI:10.3204/pubdb-2019-00117